Self-consistent bulge/disk/halo galaxy dynamical modeling using integral field kinematics

We introduce a method for modeling disk galaxies designed to take full advantage of data from integral field spectroscopy (IFS). The method fits equilibrium models to simultaneously reproduce the surface brightness, rotation, and velocity dispersion profiles of a galaxy. The models are fully self-co...

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Bibliographic Details
Main Authors:	Taranu, DS, Obreschkow, D, Dubinski, JJ, Fogarty, LMR, van de Sande, J, Catinella, B, Cortese, L, Moffett, A, Robotham, ASG, Allen, JT, Bland-Hawthorn, J, Bryant, JJ, Colless, M, Croom, SM, D'Eugenio, F, Davies, RL, Drinkwater, MJ, Driver, SP, Goodwin, M, Konstantopoulos, IS, Lawrence, JS, Lopez-Sanchez, AR, Lorente, NPF, Medling, AM, Mould, JR, Owers, MS, Power, C, Richards, SN, Tonini, C
Format:	Journal article
Published:	Institute of Physics 2017

Self-consistent bulge/disk/halo galaxy dynamical modeling using integral field kinematics

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